batgrbproduct analysis for trigger=441454

batgrbproduct Analysis for Trigger=441454

Analysis Summary

Notes:

1) No attempt has been made to eliminate the non-significant decimal places.
2) This batgrbproduct analysis is done using the HEASARC data.
3) This batgrbproduct analysis is using the flight position for the mask-weighting calculation.

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.46
    Process Start Time (local time): Tue Jan 14 01:07:09 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger441454
======================================================================

  Trigger: 00441454      Segment: 000

  BAT Trigger Time: 315687152   [s; MET]
      Trigger Stop: 315687216   [s; MET]
               UTC: 2011-01-02T18:52:25.474700    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 245.879070553938   Dec: 7.619220658419  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    11.29
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    11.29

  Flight Position:   [ source = BAT ]
    RA: 245.879070553938   Dec: 7.619220658419  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 245.878842666235   Dec: 7.61342432181446  [deg; J2000]  
        { 16h 23m 30.9s , +07d 36' 48.3" }
         +/- 1.8365543189328 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.799908740535413 [arcmin] (formal 1-sigma fit error)
    SNR: 12.7635100884259
 
  Angular difference between Flight and Ground position is 0.348044 arcmin
 
  Partial Coding Fraction: 0.6640625    [ including projection effects ]

  Duration
     T90: 265.915999948978 +/- 6.70215250002666
        Measured from: 5.05199998617172
                   to: 270.96799993515     [s; relative to TRIGTIME]
     T50: 81.1959999799728 +/- 2.31890315406829
        Measured from: 136.931999981403
                   to: 218.127999961376     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 208.759999990463     
                   to: 209.759999990463     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -58.9840000271797     
                   to: 294.824000000954     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     7.292530   9.615733   7.434354   1.828073
           0.131501   0.130169   0.114802   0.097074 [error]
 Peak      0.226939   0.354623   0.338109   0.114850
           0.009378   0.010825   0.010784   0.008124 [error]

     [ fluence units of on-axis counts / fully illuminated detector ] 

======================================================================
 
=== Fluence/Peak Flux Summary ===
 
              Model    Band1    Band2    Band3    Band4    Band5    Total      
                       15-25    25-50   50-100  100-350   15-150   15-350   keV
Fluence   Power-law 2.13e-06 3.91e-06 5.53e-06 1.64e-05 1.58e-05 2.80e-05   erg/cm2
              Error 9.01e-08 9.33e-08 1.26e-07 9.06e-07 3.11e-07 9.48e-07   erg/cm2
Peak flux Power-law 2.01e+00 2.45e+00 2.16e+00 3.28e+00 7.77e+00 9.90e+00   ph/cm2/s
              Error 1.41e-01 1.01e-01 8.65e-02 2.89e-01 2.75e-01 3.63e-01   ph/cm2/s
 
Fluence   Cutoff-PL 2.14e-06 3.92e-06 5.54e-06 1.63e-05 1.58e-05 2.79e-05   erg/cm2
              Error 7.13e-08 9.09e-08 1.18e-07 1.65e-06 3.09e-07 --------   erg/cm2
Peak flux Cutoff-PL 2.02e+00 2.45e+00 2.16e+00 3.25e+00 7.76e+00 9.87e+00   ph/cm2/s
              Error 1.52e-01 9.90e-02 -------- -------- 2.74e-01 5.41e-01   ph/cm2/s
 
Fluence        Band -------- -------- -------- -------- -------- --------   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux      Band -------- -------- -------- -------- -------- --------   ph/cm2/s
              Error -------- -------- -------- -------- -------- --------   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.500    0.039    -      -           4.71e-03 9.05e-05   46.020 57
CPL   1.497    0.057    9997.9    0.0      4.73e-03 3.45e-04   46.040 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.182    0.063    -      -           6.63e-02 2.27e-03   52.530 57
CPL   1.168    0.140    9955.1    0.0      6.73e-02 2.28e-03   52.810 56
 
Model      : spectral model: simple power-law (PL) and cutoff power-law (CPL)
Ph_index   : photon index: E^-{Ph_index} (minus sign is not included in the index)
Ph_90err   : 90% error of the photon index
Epeak      : Epeak in keV
Epeak_90err: 90% error of Epeak
Norm       : normalization at 50 keV in PL model and at 1 keV in CPL model
Nomr_90err : 90% error of the normalization
chi2       : Chi-Squared
dof        : degree of freedom

 
=== T90/T50 calculation in the 50-300 keV band (BATSE band) using 64 ms lc ===
 
T90 in the 50-300 keV band: 197.568000 sec.
T50 in the 50-300 keV band: 74.176000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100  353.808  -58.984  294.824
T90   265.916    5.052  270.968
T50    81.196  136.932  218.128
Peak    1.000  208.760  209.760

Click here for the BAT GCN circular template

Image

Pre-slew 15.0-350.0 keV image (Event data)

#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  245.8788     7.6134   0.0151    36.9120   -14.9387         1.8501323     12.764 TRIG_00441454                 
 
Foreground time interval of the image:
 -9.099  73.101 (delta_t =  82.200 [sec])
Background time interval of the image:

Lightcurves

Notes:

1) The mask-weighted light curves are using the flight position.
2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
3) For all the mask-weighted lightcurves, the y-axis units are counts/sec/det where a det is 0.4 x 0.4 = 0.16 sq cm.
4) The verticle lines correspond to following: green dotted lines are T50 interval, black dotted lines are T90 interval, blue solid line(s) is a spacecraft slew start time, and orange solid line(s) is a spacecraft slew end time.
5) Time of each bin is in the middle of the bin.

1 s binning

From T0-310 s to T0+310 s

From T100_start - 20 s to T100_end + 30 s

Full time interval

64 ms binning

Full time interval

From T100_start to T100_end

From T0-5 sec to T0+5 sec

16 ms binning

From T100_start-5 s to T100_start+5 s

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

8 ms binning

From T100_start-3 s to T100_start+3 s

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

2 ms binning

From T100_start-1 s to T100_start+1 s

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

SN=5 or 10 sec. binning (whichever binning is satisfied first)

SN=5 or 10 sec. binning (T < 200 sec)

Quad-rate summed light curves (from T0-300s to T0+1000s)

The mask-weighted light curves based on cleaned DPHs

Spectral Evolution

Spectra

Notes:

1) The fitting includes the systematic errors.
2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using the pre-slew DRM will introduce some errors in both a spectral shape and a normalization if the PHA file contains a lot of the slew/post-slew time interval.
3) For fits to more complicated models (e.g. a power-law over a cutoff power-law), the BAT team has decided to require a chi-square improvement of more than 6 for each extra dof.

Time averaged spectrum fit using the average DRM

Power-law model

Time interval is from  -58.984 sec. to  294.824 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.50031     ( -0.038551   0.0384863 )
Norm@50keV  : 4.71434E-03    ( -9.04974e-05   9.04752e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.02 using 59 PHA bins.
# Reduced chi-squared =         0.8074 for     57 degrees of freedom 
# Null hypothesis probability =   8.507218e-01
 
Photon flux (15-150 keV)    in 353.8 sec: 0.588583 ( -0.0132571  0.0133128 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.5822e-05 ( -3.11275e-07  3.11575e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from  -58.984 sec. to  294.824 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.49744     ( -0.0744348   0.0387744 )
Epeak [keV] : 9997.88      ( -9998.2 -9998.2 )
Norm@50keV  : 4.72840E-03    ( -9.0422e-05   0.000599772 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.04 using 59 PHA bins.
# Reduced chi-squared =         0.8222 for     56 degrees of freedom 
# Null hypothesis probability =   8.262488e-01
 
Photon flux (15-150 keV)    in 353.8 sec: 0.588348 ( -0.013175  0.012934 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.58213e-05 ( -3.08266e-07  3.09327e-07 ) ergs/cm2

Band function

Time interval is from  -58.984 sec. to  294.824 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.582744   ( 1.0027   1.0027 )
beta        : -1.50907    ( -0.0478749   0.0418282 )
Epeak [keV] : 40.2409      ( -40.2345 113.959 )
Norm@50keV   : 2.16403E-02    ( -0.0217608   406473 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.22 using 59 PHA bins.
# Reduced chi-squared =         0.8221 for     55 degrees of freedom 
# Null hypothesis probability =   8.237867e-01
 
Photon flux (15-150 keV)    in 353.8 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 17.7918  (  )
R^2/D10^2   : 3.46489E-02  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         651.73 using 59 PHA bins.
# Reduced chi-squared =         11.434 for     57 degrees of freedom 
# Null hypothesis probability =  7.370357e-102
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.798e-07   3.167e-08
25- 50  3.575e-06   1.033e-07
50-150  8.189e-06   2.565e-07
15-150  1.254e-05   2.707e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 2.41504       (-0.0462855     0.0462852)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          78.77 using 59 PHA bins.
# Reduced chi-squared =          1.382 for     57 degrees of freedom 
# Null hypothesis probability =   2.964496e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.128e-06   4.936e-08
25- 50  4.093e-06   8.845e-08
50-150  8.977e-06   1.857e-07
15-150  1.520e-05   3.396e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.47775        (-0.531881      0.562707)
R1^2/D10^2  : 0.482185        (-0.109691      0.149966)
kT2 [keV]   : 30.0072        (-2.07426      2.53441)
R2^2/D10^2  : 4.75256E-03    (-0.00115507   0.00136213)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.63 using 59 PHA bins.
# Reduced chi-squared =          1.030 for     55 degrees of freedom 
# Null hypothesis probability =   4.141157e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.870e-06   1.242e-07
25- 50  3.994e-06   1.574e-07
50-150  9.822e-06   4.016e-07
15-150  1.569e-05   5.112e-07

Peak spectrum fit

Power-law model

Time interval is from  208.760 sec. to  209.760 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.18170     ( -0.0635529   0.0634179 )
Norm@50keV  : 6.63204E-02    ( -0.00226863   0.00226857 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.53 using 59 PHA bins.
# Reduced chi-squared =         0.9216 for     57 degrees of freedom 
# Null hypothesis probability =   6.432201e-01
 
Photon flux (15-150 keV)    in 1 sec: 7.76521 ( -0.274735  0.275104 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.76373e-07 ( -2.59862e-08  2.6096e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from  208.760 sec. to  209.760 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.16775     ( -0.214032   0.0655719 )
Epeak [keV] : 9955.11      ( -9999.35 -9999.35 )
Norm@50keV  : 6.72577E-02    ( -0.0022617   0.00229688 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.81 using 59 PHA bins.
# Reduced chi-squared =         0.9430 for     56 degrees of freedom 
# Null hypothesis probability =   5.964819e-01
 
Photon flux (15-150 keV)    in 1 sec: 7.76494 ( -0.27633  0.27237 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.76176e-07 ( -1.374e-08  2.6156e-08 ) ergs/cm2

Band function

Time interval is from  208.760 sec. to  209.760 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.454541   ( 0.798557   5.77692 )
beta        : -1.19374    ( -0.658585   0.0697728 )
Epeak [keV] : 55.4322      ( -55.6466 309.415 )
Norm@50keV   : 0.222735    ( -0.227937   3.54048e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.12 using 59 PHA bins.
# Reduced chi-squared =         0.9477 for     55 degrees of freedom 
# Null hypothesis probability =   5.853090e-01
 
Photon flux (15-150 keV)    in 1 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 19.6184  (  )
R^2/D10^2   : 0.375026  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         245.15 using 59 PHA bins.
# Reduced chi-squared =         4.3010 for     57 degrees of freedom 
# Null hypothesis probability =   3.524779e-25
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.803e-08   1.885e-09
25- 50  1.379e-07   7.000e-09
50-150  3.922e-07   2.425e-08
15-150  5.581e-07   2.495e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (      )
Norm        : 32.0754       (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         152.60 using 59 PHA bins.
# Reduced chi-squared =         2.6771 for     57 degrees of freedom 
# Null hypothesis probability =   1.159288e-10
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.987e-08   2.995e-09
25- 50  1.536e-07   5.550e-09
50-150  3.370e-07   1.215e-08
15-150  5.705e-07   2.135e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.85055        (-1.01208      1.14038)
R1^2/D10^2  : 4.56736        (-1.57874      2.66598)
kT2 [keV]   : 34.6133        (-4.33445      6.50121)
R2^2/D10^2  : 5.21315E-02    (-0.0212513   0.0279386)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.29 using 59 PHA bins.
# Reduced chi-squared =          1.005 for     55 degrees of freedom 
# Null hypothesis probability =   4.635995e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.909e-08   7.325e-09
25- 50  1.430e-07   1.115e-08
50-150  4.790e-07   5.405e-08
15-150  6.811e-07   6.630e-08

Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)

Power-law model

 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.66541     ( -0.22431   0.229222 )
Norm@50keV  : 1.32012E-03    ( -0.000177046   0.000174092 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.27 using 59 PHA bins.
# Reduced chi-squared =          1.215 for     57 degrees of freedom 
# Null hypothesis probability =   1.277376e-01
 
Photon flux (15-150 keV)    in 82.2 sec: 0.173262 ( -0.0218356  0.0218766 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.00771e-06 ( -1.41993e-07  1.43931e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.67201     ( -0.231174   0.225191 )
Epeak [keV] : 9999.36      ( -9999.35 -9999.36 )
Norm@50keV  : 1.31736E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.27 using 59 PHA bins.
# Reduced chi-squared =          1.237 for     56 degrees of freedom 
# Null hypothesis probability =   1.095751e-01
 
Photon flux (15-150 keV)    in 82.2 sec: 0.173272 ( -0.021891  0.021796 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.00584e-06 ( -7.31827e-08  1.43686e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.64731   ( -4.64731   -4.64731 )
beta        : -1.76634    ( -0.287061   0.259773 )
Epeak [keV] : 23.8153      ( -23.8153 5.66681 )
Norm@50keV   : 119.417    ( -14.6865   972791 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.25 using 59 PHA bins.
# Reduced chi-squared =          1.241 for     55 degrees of freedom 
# Null hypothesis probability =   1.081397e-01
 
Photon flux (15-150 keV)    in 82.2 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2

S(25-50 keV) vs. S(50-100 keV) plot

S(25-50 keV)  = 3.91e-06
S(50-100 keV) = 5.53e-06

T90 vs. Hardness ratio plot

T90                                   = 265.915999948978 sec.
Hardness ratio (energy fluence ratio) = 1.41432

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.31857
Count Ratio (50-100 keV) / (15-25 keV) = 1.01945

Mask shadow pattern

IMX = 7.257620045731079E-01, IMY = 1.936348075317588E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

Spacecraft aspect plot

Bright source in the pre-burst/pre-slew/post-slew images

Pre-burst image of 15-350 keV band

Time interval of the image:

Pre-slew background subtracted image of 15-350 keV band

Time interval of the image:
-9.099400 73.100600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9902 -15.6055    3.3  53.8  -37.9   1.8881   3.5    2.2	Sco X-1                       
254.4692  35.3669    1.9  22.9   38.5   0.7408   6.1    1.6	Her X-1                       
268.3198  -1.3382    4.0  29.9  -57.7   0.4281   2.9    7.4	SW J1753.5-0127               
273.8424 -13.9062    0.0  40.9  -72.1  -0.2193  -0.6   12.3	GX 17+2                       
288.7450  10.8765    3.1  18.1 -111.5   0.4138   3.7    5.2	GRS 1915+105                  
299.6421  35.1986    1.1  19.4  158.8   1.1872  11.0    2.5	Cyg X-1                       
307.9208  41.0090   17.8  27.6  151.3  -0.0961  -0.6    9.2	Cyg X-3                       
326.0396  38.2630   12.4  40.7  161.3   0.2089   0.9    7.1	Cyg X-2                       
245.8788   7.6135    0.9  36.9  -14.9   1.8500  12.8 ------	UNKNOWN                       
320.7316  11.9335    3.5  41.6 -157.6   0.5922   3.3 ------	UNKNOWN                       
290.2195   2.5300    2.4  26.3 -105.5   0.6727   4.9 ------	UNKNOWN                       
249.0754 -16.2912    3.1  52.0  -42.3   2.3800   4.4 ------	UNKNOWN                       
248.8644 -16.3305    3.5  52.1  -42.1   2.5454   4.6 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
137.500590 963.062100
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9782 -15.6400    0.3  23.2  -38.5  28.2598  45.2    0.1	Sco X-1                       
254.4717  35.3670    1.7  28.9  153.9   5.8933   6.7    1.6	Her X-1                       
256.2217 -37.8135    7.2  46.4  -52.0  -4.0499  -1.6   11.3	4U 1700-377                   
256.3848 -36.5226    5.0  45.2  -52.6   4.9974   2.3    6.4	GX 349+2                      
263.0661 -24.7635    2.9  36.4  -67.6   4.9763   4.0    3.3	GX 1+4                        
268.3510  -1.4781    1.7  24.2 -109.6   4.6373   6.8    1.8	SW J1753.5-0127               
270.3773 -25.1240    5.8  40.5  -76.1   4.1686   2.0    5.7	GX 5-1                        
270.3893 -25.6552    9.9  40.9  -75.6   2.5000   1.2    7.1	GRS 1758-258                  
273.9841 -14.0326    5.5  35.3  -93.0   2.5060   2.1    1.3	GX 17+2                       
288.7727  11.0020    2.7  42.4 -138.8   4.8262   4.3    3.7	GRS 1915+105                  
299.7260  35.3102    9.4  56.4 -168.5   3.0757   1.3    9.3	Cyg X-1                       
262.8285 -33.8984   14.8  44.5  -60.9   1.7741   0.8    8.9	GX 354-0                      
222.0962  42.6694    2.2  40.9  112.3  13.8420   5.1 ------	UNKNOWN                       
206.2260 -32.5968    3.5  55.1    0.2   8.5025   3.3 ------	UNKNOWN                       
245.8649   7.6188    0.3   0.0  106.7  20.0237  33.9 ------	UNKNOWN                       
298.3225  37.9605    2.5  56.1 -171.9  11.2703   4.6 ------	UNKNOWN                       
216.0965 -45.6954    3.2  59.6  -17.0  12.5563   3.6 ------	UNKNOWN

Plot creation:
Sat May 30 23:15:40 EDT 2015